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19962005
most citedDo weak magnetic fields prevent hydrogen from accreting onto metal-line white dwarf stars?

24 citations · 44 across the 4 of their papers we have counts for

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astro-ph200520 cited

A NICMOS Direct Imaging Search for Giant Planets around the Single White Dwarfs in the Hyades

S. Friedrich, H. Zinnecker, W. Brandner +2

We report preliminary results from our search for massive giant planets (6-12 Jupiter masses) around the known seven single white dwarfs in the Hyades cluster at sub-arcsec separat…

astro-ph2004

Do Magnetic Fields Prevent Hydrogen from Accreting onto Cool Metal-line White Dwarf Stars?

S. Friedrich, S. Jordan, D. Koester

It is generally assumed that metals detected in the spectra of a few cool white dwarfs cannot be of primordial origin and must be accreted from the interstellar medium. However, th…

astro-ph2004

Discovery of magnetic fields in hot subdwarfs

S. J. O'Toole, S. Jordan, S. Friedrich +1

We present initial results of a project to measure mean longitudinal magnetic fields in a group of sdB/OB/O stars. The project was inspired by the discovery of three super-metal-ri…

astro-ph200424 cited

Do weak magnetic fields prevent hydrogen from accreting onto metal-line white dwarf stars?

Susanne Friedrich, Stefan Jordan, Detlev Koester

The widely accepted assumption is that metals detected in the spectra of a few cool helium-rich white dwarfs cannot be of primordial origin and therefore must be accreted from the…

astro-ph2000

Cool helium-rich white dwarfs from the Hamburg/ESO Survey

S. Friedrich, D. Koester, N. Christlieb +2

We present an analysis of 40 cool helium-rich white dwarfs found in the Hamburg/ESO survey. They were selected for follow-up spectroscopy because of their U-B colour below -0.18, t…

astro-ph1996

The Seyfert Galaxy NGC 6814 -- a highly variable X-ray source

Michael Koenig, Susanne Friedrich, Ruediger Staubert +1

The Seyfert galaxy NGC 6814 is a highly variable X-ray source despite the fact that it has recently been shown not to be the source of periodic variability. The 1.5 year monitoring…